Theia 2139

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0.24 UTI
0.0
CN
0.44
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2139 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 201.747 -62.03 0.289 -5.675 -1.744 -99.813
Hunt & Reffert 2024 201.65 -62.024 0.29 -5.621 -1.775 -74.446
Cavallo et al. 2024 202.059 -62.084 0.289 – – –
Hunt & Reffert 2023 201.65 -62.024 0.29 -5.621 -1.775 -74.446

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 495* – –
Cavallo et al. 2024 2.56 2.74 – 52 -0.050 – – –
Hunt & Reffert 2023 3.19 2.86 2.54 11 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4031 32.0 202.08 -62.07 0.3 -5.59 -1.77 -36.14 0.11

💡 Note: The % column shows the percentage of members that Theia 2139 shares with each listed object.

Visualization

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